Simulations of Al XIII-Fe XXIV X-ray laser photopumping scheme
JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER 71:2-6 (2001) 129-138
Statistical mechanics
Oxford University Press, USA, 2001
Abstract:
The present book is a teaching text designed to introduce the fundamentals of thesubject of statistical mechanics.Ultrahigh-intensity laser-produced plasmas as a compact heavy ion injection source
IEEE Transactions on Plasma Science 28:4 (2000) 1110-1115
Abstract:
The possibility of using high-intensity laser-produced plasmas as a source of energetic ions for heavy ion accelerators is addressed. Experiments have shown that neon ions greater than 6 MeV can be produced from gas jet plasmas, and well-collimated proton beams greater than 20 MeV have been produced from highintensity laser solid interactions. The proton beams from the back of thin targets appear to be more collimated and reproducible than are high-energy ions generated in the ablated plasma at the front of the target and may be more suitable for ion injection applications. Lead ions have been produced at energies up to 430 MeV. © 2000 IEEE.Three-dimensional magnetohydrodynamic numerical simulations of cloud-wind interactions
Astrophysical Journal 543:2 PART 1 (2000) 775-786
Abstract:
We present results from three-dimensional numerical simulations investigating the magnetohydrodynamics of cloud-wind interactions. The initial cloud is spherical, while the magnetic field is uniform and transverse to the cloud motion. A simplified analytical model that describes the magnetic energy evolution in front of the cloud is developed and compared with simulation results. In addition, it is found that the interaction of the cloud with a magnetized interstellar medium results in the formation of a highly structured magnetotail. The magnetic flux in the wake of the cloud organizes into flux ropes, and a reconnection current sheet is developed as field lines of opposite polarity are brought close together near the symmetry axis. At the same time magnetic pressure is strongly enhanced at the leading edge of the cloud from the stretching of the field lines that occurs there. This has an important dynamical effect on the subsequent evolution of the cloud, since some unstable modes tend to be strongly enhanced.22pWE-10 高速点火研究3 : High density relatlvistic electron propagation in high density plasma
(2000) 155